扰动重力场影响下远程车辆基于学习的多级碰撞点预测方法

IF 6.5 1区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Leliang Ren, Yong Xian, Shaopeng Li, Daqiao Zhang, Bing Li, Weilin Guo
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引用次数: 0

摘要

扰动重力场对远程车辆撞击点的影响日益突出,是影响撞击点预测精度的重要因素。为了实现干扰重力场影响下lrv的高精度快速IPP,提出了一种数据驱动的多级IPP方法,以平衡预测精度和实时性。首先,基于椭圆弹道理论预测当前飞行状态的弹着点,并计算椭圆弹道的撞击偏差(ID-ET);在第二层和第三层,分别建立神经网络模型,学习J2项和再入气动阻力以及扰动重力场引起的ID-ET。为了提高神经网络的预测性能,采用辅助圆对ID-ET进行解耦。为了降低神经网络学习的难度,基于课程学习的思想设计了一种训练策略,提高了训练的准确性。同时,提出了一种混合样本生成策略来提高神经网络的泛化能力。通过详细的仿真实验,分析了该方法的优点和计算复杂度。仿真结果表明,该模型在扰动重力场和再入气动阻力影响下具有较高的预测精度、较强的泛化能力和较好的实时性。在训练集和测试集包含的317360个样本中,3σ预测误差为6.21 m。在STM32F407单片机上,IPP需要3.415 ms。该方法可为制导算法的设计提供支持,适用于工程实践。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Learning-based multi-level impact point prediction method for long-range vehicles under the influence of a disturbing gravity field

The influence of a disturbing gravity field on the impact points of long-range vehicles (LRVs) has become increasingly prominent, which is an important factor affecting the accuracy of impact point prediction (IPP). To achieve high-accuracy and fast IPP for LRVs under the influence of a disturbing gravity field, a data-driven multi-level IPP method is proposed to balance the prediction accuracy and real-time performance. At the first level, the impact point of the current flight state is predicted based on elliptical trajectory theory, and the impact deviation of the elliptical trajectory (ID-ET) is calculated. At the second and third levels, a neural network (NN) model is established to learn the ID-ET caused by the J2 term and re-entry aerodynamic drag as well as that caused by the disturbing gravity field. To improve the NN prediction performance, an auxiliary circle is applied to decouple the ID-ET. To reduce the difficulty of NN learning, a training strategy is designed based on the idea of curriculum learning, which improves training accuracy. At the same time, a hybrid sample generation strategy is proposed to improve the NN generalization ability. A detailed simulation experiment is designed to analyze the advantages and computational complexity of the proposed method. The simulation results showed that the proposed model has a high prediction accuracy, strong generalization ability, and good real-time performance under the influence of the disturbing gravity field and re-entry aerodynamic drag. Among the 317,360 samples contained in the training and test sets, the 3σ prediction error was 6.21 m. On an STM32F407 single-chip microcomputer, the IPP required 3.415 ms. The proposed method can provide support for the design of guidance algorithms and is applicable to engineering practice.

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来源期刊
Astrodynamics
Astrodynamics Engineering-Aerospace Engineering
CiteScore
6.90
自引率
34.40%
发文量
32
期刊介绍: Astrodynamics is a peer-reviewed international journal that is co-published by Tsinghua University Press and Springer. The high-quality peer-reviewed articles of original research, comprehensive review, mission accomplishments, and technical comments in all fields of astrodynamics will be given priorities for publication. In addition, related research in astronomy and astrophysics that takes advantages of the analytical and computational methods of astrodynamics is also welcome. Astrodynamics would like to invite all of the astrodynamics specialists to submit their research articles to this new journal. Currently, the scope of the journal includes, but is not limited to:Fundamental orbital dynamicsSpacecraft trajectory optimization and space mission designOrbit determination and prediction, autonomous orbital navigationSpacecraft attitude determination, control, and dynamicsGuidance and control of spacecraft and space robotsSpacecraft constellation design and formation flyingModelling, analysis, and optimization of innovative space systemsNovel concepts for space engineering and interdisciplinary applicationsThe effort of the Editorial Board will be ensuring the journal to publish novel researches that advance the field, and will provide authors with a productive, fair, and timely review experience. It is our sincere hope that all researchers in the field of astrodynamics will eagerly access this journal, Astrodynamics, as either authors or readers, making it an illustrious journal that will shape our future space explorations and discoveries.
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